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Quantum–classical transition in scale relativity

Marie-Noëlle Célérier and Laurent Nottale

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The theory of scale relativity provides a new insight into the origin of fundamental laws in physics. Its application to microphysics allows us to recover quantum mechanics as mechanics on a non-differentiable (fractal) spacetime. The Schrödinger and Klein–Gordon equations are demonstrated as geodesic equations in this framework. A development of the intrinsic properties of this theory, using the mathematical tool of Hamilton's bi-quaternions, leads us to a derivation of the Dirac equation within the scale-relativity paradigm. The complex form of the wavefunction in the Schrödinger and Klein–Gordon equations follows from the non-differentiability of the geometry, since it involves a breaking of the invariance under the reflection symmetry on the (proper) time differential element (ds ↔ −ds). This mechanism is generalized for obtaining the bi-quaternionic nature of the Dirac spinor by adding a further symmetry breaking due to non-differentiability, namely the differential coordinate reflection symmetry (dxμ ↔ −dxμ) and by requiring invariance under the parity and time inversion. The Pauli equation is recovered as a non-motion-relativistic approximation of the Dirac equation.


PACS

03.65.Pm Relativistic wave equations

03.30.+p Special relativity

03.65.Ge Solutions of wave equations: bound states

MSC

83C10 Equations of motion

81Q50 Quantum chaos (See also 37Dxx)

81R40 Symmetry breaking

81Q05 Closed and approximate solutions to the Schrödinger, Dirac, Klein-Gordon and other quantum-mechanical equations

Subjects

Gravitation and cosmology

Quantum information and quantum mechanics

Dates

Issue 3 (23 January 2004)

Received 3 June 2003

Published 7 January 2004



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